Whitworth, Anthony Peter ORCID: https://orcid.org/0000-0002-1178-5486
1991.
Why do stars become giants?
Annales de Physique
16
(4)
, pp. 515-526.
10.1051/anphys:01991001604051500
|
Official URL: http://dx.doi.org/10.1051/anphys:01991001604051500
Abstract
In this paper I explain why stars become giants; and I review earlier work, indicating why there has been so little consensus on this question despite over fifty years of investigation. The mechanism causing giantness is not simple. It involves a complex natural conspiracy in which there are four critical roles. These roles are played by eight different physical effects
| Item Type: | Article |
|---|---|
| Date Type: | Publication |
| Status: | Published |
| Schools: | Schools > Physics and Astronomy |
| Subjects: | Q Science > QB Astronomy |
| Uncontrolled Keywords: | giant stars; stellar evolution; stellar structure; giant stars formation; stellar evolution; stellar structure equations singular behaviour; giant stars envelopes; stellar core mass; Schonberg Chandrasekhar limit; stellar mass loss; critical core structure; degenerate cores; non degenerate cores; physical effects; He core mass; stellar He ignition |
| Publisher: | EDP sciences |
| ISSN: | 0003-4169 |
| Last Modified: | 24 Oct 2022 11:19 |
| URI: | https://orca.cardiff.ac.uk/id/eprint/47736 |
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